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Diabatic processes and the structure of the warm conveyor belt
Oscar Martínez-Alvarado
J. Chagnon, S. Gray, R. Plant, J. Methven
Department of Meteorology
University of Reading
H. Joos, M. Bötcher, H. Wernli
ETH Zurich
2nd European Windstorm Workshop
Leeds, 3-4 September 2012
• Diabatic processes are fundamental to clouds and
precipitation (i.e., weather)
• In NWP models these processes are parameterized
• The nonlinear feedback between the cloud scale and
larger-scale dynamics has implications for:
Forecasts of heavy precipitation and high wind events
Assimilation of high resolution data (e.g., radar)
Linking forecast error to model representation of processes
Diabatic (heating) effects on medium-range forecasts
Design of perturbed physics ensembles
Why study diabatic processes in ET storms?
Systematic error (PV overestimated) in medium-range
weather forecasts on the downstream side of troughs.
Diabatic PV near the tropopause
Objectives
• Evaluate the accuracy of numerical models in
simulating atmospheric diabatic processes
– Extratropical cyclones and more specifically the warm
conveyor belt (WCB) constitute the focus of this study
• What diabatic processes act on the WCB?
• What effect do these processes have on the WCB
development?
• What are the consequences for the subsequent
development of the upper-level atmospheric structure?
Warm conveyor
belt
Satellite image courtesy of NERC Satellite Receiving Station,
Dundee University, Scotland http://www.sat.dundee.ac.uk
Surface fronts based on the Met Office analysis at 00 UTC 25
Nov 2009 (archived by http://www.wetter3.de/fax)
Cyclone’s low
pressure centre
Cold conveyor
belt
Channel 22, satellite
Aqua
0247 UTC 25 Nov 2009
Methods
0
proc
( , )( , ) ( , )i
i
x t xt tx
Tracers (I)
Tracers (II)
·
i
i ii
DS
Dt t
v
0 00
· 0
D
Dt t
v
The conserved field is
affected by advection
only
= proc = p
0
roc
· ·
ii
i i
St
v v
Total rate of change
Advection of
conserved field
Advection of accumulated
tendencies
Sources
Consistency between tracers
and trajectories
Numerical models and
simulations
• Two numerical weather forecast models have been
used
• Reading: The Met Office Unified Model (MetUM)
– 12 km resolution
• ETH-Zürich: The COSMO (COnsortium for Small-scale
Modelling) model
– 14 km resolution
• Both simulations initialised at 0600 UTC 23 November
2009 from ECMWF operational analysis fields.
Case-study:
Synoptic-scale context
• The surface low formed in the North Atlantic on 23 November 2009 along an
east-west oriented baroclinic zone
• The low deepened from 0000 UTC 23 November to 0000 UTC 25 November
2009 and moved eastward.
• By 0000 UTC 25 November, the system was occluded and had undergone
“frontal fracture”.
• Precipitation was heavy and continuous along the length of the cold front
during the period 23-25 November 2009. As such, this is an ideal case for
examining diabatic heating in a WCB.
• The upper-level trough associated with the primary low amplified in concert
with the surface low.
• The downstream ridge and downstream trough also amplified during this
period.
Trajectory selection
Wide starting
region to capture
every ascending
trajectory related
to the system
A
B
C
Trajectory bundle
Identification of sub-streams
θ < 307.5 K θ > 307.5 K
X grid point X grid point X grid point
Y g
rid
poin
t
All trajectories
Lower branch Upper branch
B + C A
Potential temperature conserved
component (K)
Model level at 9.68 km
Upper-level structure (I)
Potential temperature (K)
Diabatic potential vorticity (PVU) Diabatic potential temperature
(K)
1
0.5
0
-0.5
2
Model level at 9.68 km
Upper-level structure (II)
A B + C
D
Dt
(K h
-1)
Pressure
(hPa)
Pressure
(hPa)
lscD
Dt
(K h
-1)
Heating rates – MetUM (I)
Total
heating
Total
heating
Large-
scale cloud Large-
scale cloud
A B + C
D
Dt
(K h
-1)
(K h
-1)
Heating rates – MetUM (II)
Pressure
(hPa)
Pressure
(hPa)
bllhD
Dt
Total
heating
Total
heating
Boundary
layer Boundary
layer
A B + C
D
Dt
(K h
-1)
(K h
-1)
Heating rates – MetUM (III)
Pressure
(hPa)
Pressure
(hPa)
convD
Dt
Total
heating
Total
heating
Convection Convection
A + B C
D
Dt
Heating rates – COSMO model
Pressure
(hPa)
Pressure
(hPa)
Summary and conclusions
• The WCB splits in two branches in its outflow region
• The upper-level structure reflects and is affected by
this split
• Diabatic processes act differently over these two
branches
• The upper-level structure is modified by these diabatic
processes (through the WCB split)
Future work
• Complete a systematic comparison between the two
models
– Further integrate the diabatic decomposition techniques at both
research centres
• The formation of a streamer at the tip of the downstream
ridge over North Africa may be noteworthy? Did this lead to
heavy precipitation downstream in the eastern Med?
– A MetUM forecast of the upper-level trough and ridge structure
only departed from the analysis in one noteworthy respect -- the
downstream ridge extended too far northwards .
– A second MetUM forecast was also performed but not discussed
here. This forecast, which was initialised 30 hours earlier, was
much less accurate than the one presented here (e.g., the
downstream ridge was not elongated and did not lead to
streamer formation)
References
• Grams, C. M., Wernli, H., Bötcher, M., Čampa, J.,
Corsmeier, U., Jones, S. C., Keller, J. H., Lenz, C.-J.
and Wiegand, L. (2011) The key role of diabatic
processes in modifying the upper-tropospheric wave
guide: a North Atlantic case-study. Q. J. R. Meteorol.
Soc. 137: 2174–2193.
• Joos, H. and Wernli, H. (2011) Influence of
microphysical processes on the potential vorticity
development in a warm conveyor belt: a case-study
with the limited-area model COSMO. Q. J. R.
Meteorol. Soc. 138: 407–418